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Astronomers Capture Earliest Stage of Planet Formation Around HOPS-315

Observations by the James Webb Space Telescope alongside ALMA revealed silicon monoxide condensing into solid grains at the asteroid-belt equivalent of the protoplanetary disk.

Diese Aufnahme des ALMA-Observatoriums zeigt heiße Gase um den Protostern HOPS-315. In seiner protoplanetaren Scheibe haben Astronomen Silikatkristalle nachgewiesen – erste Bausteine der späteren Planetesimale und Planeten. © ALMA(ESO/NAOJ/NRAO), M. McClure et al.

Overview

  • For the first time, researchers have directly detected silicon monoxide transitioning from gas to solid as the onset of planet formation around a young star.
  • The target protostar HOPS-315 lies about 1,300 light-years away in the Orion Nebula and resembles the Sun in its infancy.
  • Infrared spectra from JWST and millimeter measurements from ALMA pinpointed the condensing SiO to a ring roughly 2.2 astronomical units from HOPS-315.
  • That region mirrors the distance of our Solar System’s asteroid belt where initial rock clumps coalesce into planetesimals.
  • Scientists will use these observations to refine models of early Solar System evolution and the formation of rocky planets like Earth.